Challenges in Panchromatic Modelling with Next Generation Facilities

›9:05 (20min)

Registration open

9:05 - 9:25 (20min)

Registration open

Registration desk is open throughout the week

›9:25 (1h40)

Pushing the technical frontier: from overwhelming large datasets to machine learning
Kentaro Nagamine

9:25 - 11:05 (1h40)

Pushing the technical frontier: from overwhelming large datasets to machine learning

Kentaro Nagamine

› Integration of Semi Analytic Model with SED Modelling Platforms - Dian Triani, Swinburne University of Technology 09:25-09:45 (20min)

› Variations of the stellar initial mass function in semi-analytical models: implications for the mass assembly of galaxies in the GAEA model. - Fabio Fontanot, Astronomical Observatory of Trieste 09:45-10:05 (20min)

› Dust extinction and emission properties in a cosmological simulation - Shohei Aoyama, ASIAA 10:05-10:25 (20min)

› Simulating Galaxy Spectra with the FIRE Simulations - Tova Yoast-Hull, Canadian Institute for Theoretical Astrophysics 10:25-10:45 (20min)

› Modeling the panchromatic emission of galaxies with CIGALE - Médéric Boquien, Universidad de Antofagasta 10:45-11:05 (20min)

›11:05 (30min)

Poster session and Break

11:05 - 11:35 (30min)

Poster session and Break

›11:35 (1h40)

Pushing the technical frontier: from overwhelming large datasets to machine learning
Fangting Yuan

11:35 - 13:15 (1h40)

Pushing the technical frontier: from overwhelming large datasets to machine learning

Fangting Yuan

› Advanced panchromatic spectral modelling and fitting with BAGPIPES - Adam Carnall, Royal Observatory Edinburgh 11:35-11:55 (20min)

› FortesFit: Flexible SED modelling with a Bayesian backbone - David Rosario, Department of Physics, Durham University 11:55-12:15 (20min)

› Going beyond Galaxy Ages with Dense Basis Star Formation History Reconstruction - Kartheik Iyer, Rutgers, The State University of New Jersey 12:15-12:35 (20min)

› A Dust Spectral Energy Distribution Model with Hierarchical Bayesian Inference and Its Application to the Nearby Universe - Frédéric Galliano, UMR Astrophysique, Instrumentation-Modelisation, à Paris-Saclay 12:35-12:55 (20min)

› Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies - Yunkun Han, Yunnan Observatories, CAS 12:55-13:15 (20min)

›13:15 (4h45)

Free afternoon

13:15 - 18:00 (4h45)

Free afternoon

›19:00 (2h)

Banquet

19:00 - 21:00 (2h)

Banquet